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Table 4

Summary of APEX observations of southern sources.

Source Transition Velocity range sp. resol. Tmb(peak) rms Area rms(area) Eq. line width Comments
km s-1(LSR) km s-1 K K K km s-1 K km s-1 km s-1

AR Pup 12CO 3–2 29 ±200 0.53 0.02 ISM narrow line
12CO 2–1 29 ± 200 0.6 0.06 ISM narrow line

IRAS 08544-4431 12CO 3–2 45 ± 12 0.53 0.56 0.02 4.22 0.035 7.5
12CO 2–1 0.45 3 SEST data (Maas et al.)

IW Car 12CO 3–2 − 28 ± 9 0.53 0.22 0.03 0.71 0.035 3.2
12CO 2–1 − 28 ± 9 0.6 0.14 0.015 0.54 0.025 3.9

IRAS 10174-5704 12CO 3–2 3 ± 200 0.53 0.04 strong IS cont.
12CO 2–1 3 ± 200 0.6 0.02 strong IS cont.

IRAS 10456-5712 12CO 3–2 − 9 ± 200 0.53 0.03 strong IS cont.
12CO 2–1 − 9 ± 200 0.6 0.015 strong IS cont.

HD 95767 12CO 3–2 − 32 ± 50 1.1 0.05 0.013 0.26 0.03 5.2
12CO 2–1 − 32 ± 50 1 ~0.03 0.01 ~0.06 0.02 5.2*

RU Cen 12CO 3–2 − 35 ± 200 0.53 0.02 undetected CO em.
12CO 2–1 − 35 ± 200 0.6 0.015 undetected CO em.

HD 108015 12CO 2–1 − 2 ± 6 0.6 0.11 0.02 0.72 0.04 6.5

IRAS 15469-5311 12CO 3–2 − 14 ± 200 0.53 0.02 strong IS cont.
12CO 2–1 − 14 ± 200 0.6 0.02 strong IS cont.

IRAS 15556-5444 12CO 3–2 0 ± 200 0.53 0.02 IS contamination
12CO 2–1 0 ± 200 0.6 0.015 IS contamination

Notes. The velocity range is that occupied by the full line profile and used in particular to calculate the line area. For undetected sources, the velocity range is the total analyzed range (centered on the velocity of the source deduced from optical data). The uncertainty of the area has been calculated considering the number of spectral channels included in the equivalent line width (given in the last column, see text). An asterisk indicates value assumed from data of other lines. Uncertain values are indicated by the symbol ~.

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